Source List

Observation details report
Detailed source parameters (including errors) in a comma-separated values file

Click on source number for detailed analysis, including spectral fits if applicable

data idnum idradec telescope instrument x y cnts cntserr rate rateerr SNR poisprob sigmaj sigmin incang offax cnts_soft cnts_hard hr hr_err ext var N_H flux vign flags
Report srcpi bgdpi arf rmf 1 X202027.92+435116.0 xmm pn 322.607 296.025 73566.4 304.461 2.98399 0.0123495 531.89 1 5.93957 5.93957 0 1.77317 F T 4.17718 2.55983e-11 1 dsxf
Report srcpi bgdpi arf rmf 1 X202027.97+435116.2 xmm mos2 322.485 296.073 29769.9 199.833 1.11928 0.00751325 414.514 1 5.49953 4.89573 67.465 1.7598 F T 4.17698 3.10457e-11 1 dsxf
Report srcpi bgdpi arf rmf 1 X202028.00+435115.9 xmm mos1 322.398 296.009 20545.9 164.495 0.977985 0.00782995 254.593 1 5.87382 5.38834 334.234 1.75025 F T 4.17679 2.51869e-11 1 dsxf
Report srcpi bgdpi arf 2 X202103.70+435750.3 xmm pn 233.742 386.648 389.912 25.65 0.0158151 0.00104038 2.81909 0.997506 10.875 10.875 0 7.93094 F F 4.15016 1.12569e-13 1 dx
Report srcpi bgdpi arf rmf 3 X202103.91+435747.7 xmm mos2 233.244 386.102 122.135 16.5685 0.00459199 0.000622936 1.7006 0.955636 6.5049 6.5049 0 7.91305 F F 4.14956 1.27662e-13 1 dsx

counts and rate are bgd.-subtracted, based on simple spatial fitting (if done) or extracted counts from aperture otherwise (N.B., in either case aperture counts are given csv file).
cntserr, rateerr = Error on (source) counts and count rate, based on error in total counts
SNR = signal-to-noise ratio, computed using Nsrc/sqrt(Nbgd)
poisprob = Poisson probability of observing total counts given bgd. counts
sigmaj, sigmin = source extent (from detection output or spatial fitting) in units of arcsecs.
incang = position angle of source (inclination from x-axis)
cnts_soft = bgd.-subtracted counts in soft band (0.50 - 2.00 KeV, always taken directly from source aperture rather than model fitting)
cnts_hard = bgd.-subtracted counts in hard band (2.00 - 10.00 KeV, always taken directly from source aperture rather than model fitting)
hr, hr_err = hardness ratio ([cnts_hard-cnts_soft]/[cnts_hard+cnts_soft]) and error
ext = source extension flag: F = false (not extended), A = true (extended), A = asymetric (ratio of sigmaj/sigmin > 1 + x, where x = 0.5 by default)
var = variability flag: U = unknown, F = false (is not variable), T = true
N_H = Galactic column density as determined from LHEASOFT nh program
flux = flux determined from count rate using pimms (in the 0.30-8.00 keV bandpass for a power-law model with ph. index = 1.8)
vign = vignetting correction
Flags: d = detection parameters, s = simple spatial fitting parameters, b = simple spatial fitting failed, p = poor simple spatial fit, x = extracted events parameters, t = temporal anaylsis parameters, i = psf spatial fitting parameters, f = spectral fitting parameters, c = source is confused, u = user-defined source, v = detected source coincident with user-defined source, r = source is in region-of-interest